TAIGA Gamma Observatory: Status and Prospects

L. A. Kuzmichev; I. I. Astapov; P. A. Bezyazeekov; V. Boreyko; A. N. Borodin; N. M. Budnev; R. Wischnewski; A. Y. Garmash; A. R. Gafarov; N. V. Gorbunov; V. M. Grebenyuk; O. A. Gress; T. I. Gress; A. A. Grinyuk; O. G. Grishin; A. N. Dyachok; A. V. Zagorodnikov; V. L. Zurbanov; A. L. Ivanova; Y. A. Kazarina; N. N. Kalmykov; N. I. Karpov; V. V. Kindin; P. S. Kirilenko; S. N. Kiryuhin; V. A. Kozhin; R. P. Kokoulin; K. G. Kompaniets; E. E. Korosteleva; E. A. Kravchenko; M. Kunnas; A. Chiavassa; A. A. Lagutin; V. V. Lenok; B. K. Lubsandorzhiev; N. B. Lubsandorzhiev; R. R. Mirgazov; R. Mirzoyan; R. D. Monkhoev; R. Nachtigall; E. A. Osipova; M. I. Panasyuk; L. V. Pankov; A. L. Pakhorukov; A. A. Petrukhin; V. A. Poleschuk; M. Popesku; E. G. Popova; A. Porelli; E. B. Postnikov; V. V. Prosin; V. S. Ptuskin; A. A. Pushnin; R. I. Raikin; G. I. Rubtsov; Ya. I. Sagan; V. S. Samoliga; L. G. Sveshnikova; Yu. A. Semeney; A. Y. Sidorenkov; A. A. Silaev; A. A. Silaev; A. V. Skurikhin; M. Slunecka; A. V. Sokolov; V. P. Sulakov; V. A. Tabolenko; B. A. Tarashansky; L. G. Tkachev; A. V. Tkachenko; M. Tluczykont; O. L. Fedorov; A. D. Horns; C. Spiering; A. Sh. M. Elshoukrofy; I. I. Yashin

doi:10.1134/S1063778818040105

TAIGA Gamma Observatory: Status and Prospects

作者: Kuzmichev L.A.¹^,2, Astapov I.I.³, Bezyazeekov P.A.², Boreyko V.⁴, Borodin A.N.⁴, Budnev N.M.², Wischnewski R.⁵, Garmash A.Y.⁶^,7, Gafarov A.R.², Gorbunov N.V.⁴, Grebenyuk V.M.⁴, Gress O.A.², Gress T.I.², Grinyuk A.A.⁴, Grishin O.G.², Dyachok A.N.², Zagorodnikov A.V.², Zurbanov V.L.², Ivanova A.L.², Kazarina Y.A.², Kalmykov N.N.¹, Karpov N.I.¹, Kindin V.V.³, Kirilenko P.S.⁶, Kiryuhin S.N.², Kozhin V.A.¹, Kokoulin R.P.³, Kompaniets K.G.³, Korosteleva E.E.¹, Kravchenko E.A.⁶^,7, Kunnas M.⁸, Chiavassa A.⁹^,10, Lagutin A.A.¹¹, Lenok V.V.², Lubsandorzhiev B.K.¹², Lubsandorzhiev N.B.¹, Mirgazov R.R.², Mirzoyan R.¹³, Monkhoev R.D.², Nachtigall R.⁷, Osipova E.A.¹, Panasyuk M.I.¹, Pankov L.V.², Pakhorukov A.L.², Petrukhin A.A.³, Poleschuk V.A.², Popesku M.¹⁴, Popova E.G.¹, Porelli A.⁵, Postnikov E.B.¹, Prosin V.V.¹, Ptuskin V.S.¹⁵, Pushnin A.A.², Raikin R.I.¹¹, Rubtsov G.I.¹², Sagan Y.I.⁴, Samoliga V.S.², Sveshnikova L.G.¹, Semeney Y.A.², Sidorenkov A.Y.¹², Silaev A.A.¹, Silaev A.A.¹, Skurikhin A.V.¹, Slunecka M.⁴, Sokolov A.V.⁶^,7, Sulakov V.P.¹, Tabolenko V.A.², Tarashansky B.A.², Tkachev L.G.⁴, Tkachenko A.V.⁴, Tluczykont M.⁸, Fedorov O.L.², Horns A.D.⁸, Spiering C.⁵, Elshoukrofy A.S.¹^,16, Yashin I.I.³
隶属关系:
1. Skobeltsyn Institute of Nuclear Physics
2. Research Institute ofApplied Physics
3. National Research Nuclear University MEPhI
4. Joint Institute for Nuclear Research
5. Deutsches Elektronen-Synchrotron DESY
6. Novosibirsk State University
7. Budker Institute of Nuclear Physics, Siberian Branch
8. Institut für Experimentalphysik
9. Physics Department of the University of Torino
10. Istituto Nazionale di Fisica Nucleare
11. Altai State University
12. Institute for Nuclear Research
13. Max Planck Institute for Physics
14. Space Science Institute
15. Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
16. Damanhour University
期: 卷 81, 编号 4 (2018)
页面: 497-507
栏目: Elementary Particles and Fields
URL: https://journal-vniispk.ru/1063-7788/article/view/194361
DOI: https://doi.org/10.1134/S1063778818040105
ID: 194361

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Over the past few years, the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma-ray Astronomy) observatory has been being deployed in the Tunka Valley, Republic of Buryatia. It is designed for studying gamma rays of energy above 30 TeV and performing searches for sources of galactic cosmic rays with energies in the vicinity of 1 PeV, which is an energy region around the classic knee in the cosmic-ray energy spectrum. The first phase of the observatory will be situated at a distance of about 50 km from Lake Baikal at the site of the Tunka-133 array. The TAIGA gamma observatory will include a network of 500 wide-angle (0.6 sr) Cherenkov detectors (TAIGA-HiSCORE array) and up to 16 atmospheric Cherenkov telescopes (ACT) designed for analyzing the EAS images (imaging atmospheric Cherenkov telescopes, or IACT) and positioned within an area of 5 km². The observatory will also include muon detectors of total area 2000 m² distributed over an area of 1 km². Within the next three years, it is planned to enhance the area of the TAIGA-HiSCORE array by a factor of four—from 0.25 km² to 1 km²; to supplement the existing IACT with two new ones; and to deploy new muon detectors with a total coverage of 200 m². The structure of the new observatory is described along with the data analysis techniques used. The most interesting physical results are presented, and the research program for the future is discussed.

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TAIGA Gamma Observatory: Status and Prospects

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